CRRES卫星内部充电的模拟计算与验证

基于Geant 4软件建立一种用于计算航天器内部充电所产生电场的方法.分析载有IDM仪器的CRRES卫星当时所处的空间电子环境,使用该方法进行内部充电模拟,并将模拟结果与IDM仪器所测得的放电脉冲数据进行对比,不仅验证了该方法的有效性,更重要的是深入认识了引起航天器内部充电的空间环境特征以及材料特性对充放电效应的影响.介质内最大电场的模拟计算结果与CRRES卫星实际观测到的放电现象吻合;在材料的各项参数中,与辐射感应电导率有关的kp系数对稳态电场有很大影响,为了定量研究内部充电效应,需要在实验室精确地测定kp系数;材料的暗电导率、密度以及材料的分子构成等也与内部充电效应有关,对这些参数细致地研究有助于对内部充电效应的认识.      

Robust trajectory planning for UAV communication systems in the presence of jammers

Unmanned Aerial Vehicle(UAV) has emerged as a promising novel application for the Sixth-Generation(6G) wireless communication by leveraging more favorable Line-of-Sight(Lo S)propagation. However, the jamming resistance by exploiting UAV’s mobility is a new challenge in the UAV-ground communication. This paper investigates the trajectory planning problem in an UAV communication system, where the UAV is operated by a Ground Control Unit(GCU)to perform certain tasks in the presence of multiple jamm...     

稀薄流区高超声速飞行器表面缝隙流动结构及气动热环境的分子模拟

针对高空稀薄流区的高超声速飞行器表面缝隙或缺陷结构导致的局部气动加热问题,采用直接模拟Monte Carlo(DSMC) 方法研究了70、75、80km和90km等4个飞行高度下稀薄流区高超声速缝隙流动问题,考虑稀薄气体效应和三维效应对缝隙内部流场结构和热流的影响。结果表明:上述飞行高度下,外部流动的分离和再附在缝隙内部形成一个充满腔体的单涡结构;稀薄气体效应对缝隙内部流动结构和壁面热流影响明显,随着高度的增加,主涡涡心上移,其形状逐渐变得“扁长”,右上角逐渐变尖,热流越来越集中分布于缝隙下游侧面的顶部区域;三维缝隙效应阻碍来流气体分子进入缝隙,导致主涡涡心上移,二维缝隙假设会高估缝隙表面的热流。      

基于体积力模型的大S弯进气道与风扇耦合计算研究

为理解超紧凑大S弯进气道与风扇的耦合效应,基于体积力模拟方法开展了一体化计算研究。研究的进气道长径比为2.5,使用Rotor 67进行耦合分析,体积力模型与冻结转子计算得到的总压比、总温比和等熵效率分别相差4.49%,0.26%和2.38%。流场分析表明,风扇对入口段流场影响较为明显,主要体现为畸变区的顺向偏转与微弱衰减;进气道出口畸变经过风扇叶片后得到改善,大低压区和反向旋流基本消失;而流体在叶片的前后缘旋流角与轴向速度的综合改变量越大,风扇对气流做功越多。总的来说,超紧凑大S弯进气道与风扇之间耦合比较明显,需要在设计时进行详细的考察。     

冷却塔群塔刚体测压试验研究

在考虑冷却塔群塔和周围复杂建筑物场地条件下,通过冷却塔表面刚体测压试验,研究了双曲线型圆截面冷却塔表面雷诺数效应模拟、冷却塔表面气动压力分布特征;基于等效阻力系数表达式,研究了几种典型多塔组合工程场地条件下,群塔相对于单塔的等效风荷载比例系数,并进一步分析了冷却塔在最不利吹风工况中,位移、主拉、压应力分布关系.     

基于环路滤波器的低复杂度LMS算法设计

研究利用多天线结构对测控信号内存在的干扰进行对消和信号增强的技术。首先介绍传统空域干扰对消算法LMS，以及LMS的诸多改进算法，分析当前这些LMS算法在强干扰存在时收敛稳定性和收敛速度之间的折中关系以及参数调节的难度，分析了定步长和变步长LMS算法的优劣。针对变步长LMS由于动态环境以及大功率干扰的存在引起的收敛速度变慢和步长计算复杂的问题，提出了一种基于二阶环路滤波器累计误差的低复杂度LMS算法LF-LMS，该算法弱化单次误差的不稳定性并提高累计误差的稳定性，利用大步长和可变误差以实现快速收敛并缩小进入稳定状态后的误差波动，且计算量较小，可以有效应用于DSP工程实现，并通过仿真验证了算法在收敛速度和动态环境下的鲁棒性。     

An improved prediction model for corner stall in axial compressors with dihedral effect

Corner stall predictions are important and difficult in axial compressors. However, all of the prediction models have proved to be ineffective for advanced compressor blades, which tend to use the combined sweep and dihedral. As for the prediction parameter DL, although it effectively modeled the effects of the adverse pressure gradient and secondary flow, it failed to predict the corner stall of curved blades because the model failed to consider the intersection of the boundary layer at the corner region. In this paper, the shape factor gradient Ψ of the boundary layer at the corner region was investigated by numerically studying specially shaped expansion pipes under different adverse pressure gradients. The improved prediction parameter DJ was presented based on the model of Ψ and the circumferential pressure gradient ξ. A comparison of the critical range of the prediction parameters DL and DJ was investigated using the NACA65 cascade database, which was established by a numerical method. Then, the stall criterion was validated according to the experimental results of various test facilities with different blade geometries and experimental conditions. The results show that the improved prediction parameter is able to predict the corner separation/stall flows and is in good agreement with the experimental results for axial compressors with three-dimensional designed blades.     

Experimental of combustion instability in NTO/MMH impinging combustion chambers

This paper presents an experimental study into dynamics of chamber pressure and heat release rate during self-excited spinning and standing azimuthal mode in NTO/MMH (nitrogen tetroxide/monomethylhydrazine) impinging combustion chambers. Nine cases including two combustion chamber configurations were conducted. The operating conditions of all unstable cases were located in the instability region according to Hewitt empirical correlation. The results show that chamber pressure oscillations keep pace with the corresponding OH* chemiluminescence intensity over the whole combustion region in the spinning and standing modes. It is indicated that the Rayleigh index is positive over the whole combustion area in all the unstable cases. A significant supersonic flame front structure of the first-order spinning mode was found in a cylindrical chamber, which means that a detonation wave could exist in the cylindrical chamber without a center body. The pressure and heat release rate oscillations at the pressure node are nonnegligible although their amplitudes are lower than those at the pressure antinode in the first-order standing mode with an annular chamber. Besides, the dominant frequency of pressure and heat release rate oscillations at the pressure node is twice as high as that at the pressure antinode.     

Aero-optical effects simulation technique for starlight transmission in boundary layer under high-speed conditions

Aero-optical effects for starlight transmission in the high-speed flow field will reduce the accuracy of the star sensor on an aircraft. Numerical simulations for aero-optical effects usually require plenty of calculations, which cause difficulties when designing a celestial navigation system for a high-speed aircraft. In this study, an Aero-Optical Simulator For Starlight Transmission (AOSST) in the boundary layer is developed. It effectively reduces the computational burden compared to that of the widely used CFD simulation, and it achieves satisfactory accuracy. In this simulator, gas ellipsoids satisfying certain design rules are used to simulate coherent density structures in boundary layers. Design rules for the gas ellipsoids are found from published experimental and high-fidelity CFD simulation results. The generated wavefront distortion by AOSST is anchored with the scale law for aero-optical distortion in the boundary layer by determining some control parameters, which enables the simulator to output reliable results over a wide range of flight states. Four numerical examples are provided to verify the performance of AOSST. The results demonstrate that AOSST is able to simulate the directional dependence of aero-optical distortions in boundary layers, the variation trend of distorted wavefront shapes with Reynolds number, and the grayscale distribution on the disturbed star map.     

Calibration errors in determining slant Total Electron Content (TEC) from multi-GNSS data

The global navigation satellite system (GNSS) is presently a powerful tool for sensing the Earth's ionosphere. For this purpose, the ionospheric measurements (IMs), which are by definition slant total electron content biased by satellite and receiver differential code biases (DCBs), need to be first extracted from GNSS data and then used as inputs for further ionospheric representations such as tomography. By using the customary phase-to-code leveling procedure, this research comparatively evaluates the calibration errors on experimental IMs obtained from three GNSS, namely the US Global Positioning System (GPS), the Chinese BeiDou Navigation Satellite System (BDS), and the European Galileo. On the basis of ten days of dual-frequency, triple-GNSS observations collected from eight co-located ground receivers that independently form short-baselines and zero-baselines, the IMs are determined for each receiver for all tracked satellites and then for each satellite differenced for each baseline to evaluate their calibration errors. As first derived from the short-baseline analysis, the effects of calibration errors on IMs range, in total electron content units, from 1.58 to 2.16, 0.70 to 1.87, and 1.13 to 1.56 for GPS, Galileo, and BDS, respectively. Additionally, for short-baseline experiment, it is shown that the code multipath effect accounts for their main budget. Sidereal periodicity is found in single-differenced (SD) IMs for GPS and BDS geostationary satellites, and the correlation of SD IMs over two consecutive days achieves the maximum value when the time tag is around 4?min. Moreover, as byproducts of zero-baseline analysis, daily between-receiver DCBs for GPS are subject to more significant intra-day variations than those for BDS and Galileo.